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Transport of open magnetic flux between solar polar regions

Published online by Cambridge University Press:  26 February 2010

Alexei A. Pevtsov  and
Valentyna I. Abramenko
Alexei A. Pevtsov
Affiliation:
National Solar Observatory, Sunspot, NM 88349, U.S.A. email: apevtsov@nso.edu
Valentyna I. Abramenko
Affiliation:
Big Bear Solar Observatory, New Jersey Institute of Technology, Big Bear City, CA 92314-9672, U.S.A. email: avi@bbso.njit.edu
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Abstract

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We present the observations of coronal hole that has originated at the polar hole in one hemisphere, extended to equatorial region, got disconnected and transported across the equator to polar region of opposite hemisphere.

Keywords

Sun: magnetic fieldsSun: activitySun: coronaSun: photosphere
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Symposium S264: Solar and Stellar Variability: Impact on Earth and Planets , August 2009 , pp. 210 - 212
Copyright
Copyright © International Astronomical Union 2010

References

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